Speaker
Dr.
Helen Barminova
(NRNU MEPhI)
Description
3D self-consistent model is discussed which may describe the quasi-stable stellar system. Such model describes the system having the shape of oblate rotational ellipsoid. The common case of anisotropic "pressure" in the plane of symmetry is considered. Some aspects of quasi-relaxed states of such systems and possible system evolution are discussed shortly.
Primary author
Dr.
Helen Barminova
(NRNU MEPhI)
Co-authors
Prof.
A. Chikhachev
(SSC All-Russian Electrotechnical Institute (VEI))
